CDM models with negative pressure

Details CDM models with negative pressure CDM models with negative pressure

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hell.confe.125b&link_type=abstract

"5th Hellenic Astronomical Conference, held 20-22 September, 2001 in Crete, Greece. Online at http://www.astro.auth.gr/elaset/he

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The available high quality cosmological data (like SN Ia, CMB, ect) are well fitted by an emerging ''standard model'' which contains cold dark matter (CDM) to explain clustering and dark energy (negative pressure) to close the Universe. In this work we investigate all the neoclassical tests of the above ''standard model'' as well as its variants (Quintessence Cosmology) in order to understand better the theoretical expectations of this models and compare with the available data.

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